Light as Particles
Light as Particles
Planck quantized the energy exchanged between matter and radiation (P.2.1); Einstein, in 1905, quantized the light itself. This lesson follows the evidence that forced the photon on a reluctant physics community: the photoelectric effect, X-ray production, Compton scattering, and the creation and annihilation of matter. By the end, light — which Young's fringes had settled as a wave — is also, undeniably, a hail of particles. Light, like a cat, declines to be only one thing.
Learning Objectives
After this lesson you will be able to:
- List the experimental facts of the photoelectric effect and explain, point by point, why the classical wave picture fails on each.
- Apply Einstein's photon hypothesis to compute work functions, , and stopping potentials, and explain what Millikan's slope measures.
- Derive the photon momentum from the relativistic energy–momentum relation.
- Derive the Duane–Hunt cutoff and recognize it as the photoelectric effect in reverse.
- Derive the Compton shift from relativistic energy and momentum conservation.
- Explain the threshold and kinematics of pair production and annihilation, including why each requires (or produces) more than one body.
Intuition
Classically, light is a continuous electromagnetic wave: energy flux proportional to the squared amplitude (intensity), spread smoothly over the whole wavefront. Einstein's proposal replaces the smooth flood with rain: light of frequency arrives in discrete packets — photons — each of energy . Brightness counts how many packets arrive per second; color sets how much energy each carries; one photon is absorbed by one electron, whole or not at all. Every "impossible" photoelectric fact below becomes obvious in this picture — and the same bookkeeping, pushed through special relativity, predicts the Compton shift to four significant figures.
Theory
The photoelectric effect: the facts, and why the wave picture fails on each
Shine light on a clean metal in vacuum; electrons come off and are collected, giving a photocurrent. Four facts, established between Hertz (1887) and Millikan (1916) — each paired, point by point, with what a classical wave (energy delivered continuously, at a rate , spread over the wavefront) predicts:
- Threshold frequency. Each metal has a below which no electrons are emitted, at any intensity. Classically, any frequency should eject electrons if the light is bright enough — there should be no threshold.
- No time lag. Emission starts within , even in feeble light. Classically, an atom of radius intercepts so little of a weak wavefront that accumulating a few eV should take months (E3: 135 days).
- Intensity controls the current, not the electron energy. Doubling intensity doubles the photocurrent; is unchanged. Classically, a larger amplitude shakes electrons harder, so should grow with intensity.
- Stopping potential is linear in frequency. The reverse voltage that just stops the fastest electrons () grows linearly with , with the same slope for every metal. Classically, frequency is nearly irrelevant to energy transfer — no universal slope, let alone one equal to with the blackbody of P.2.1.
Einstein's photon and the photoelectric equation
Einstein (1905): light of frequency consists of quanta of energy , with . One photon is absorbed by one electron, which pays the work function — its minimum binding energy to the metal, a few eV — and leaves with at most
Every fact follows. Threshold: — below it no single photon suffices (and two-photon absorption is fantastically unlikely at ordinary intensities). No lag: the energy arrives in one lump. Intensity: more photons per second means more electrons per second, but each still gets exactly . And is a straight line of metal-independent slope , intercept . Millikan spent a decade trying to refute this and in 1916 confirmed it, measuring — within 0.5% of the blackbody value. Independent phenomena, same constant.
Photon momentum
Special relativity relates energy, momentum, and mass by . A photon travels at , which no massive particle can do at finite energy, so and
using . The momentum is tiny — a green photon carries (E2) — but real: it reproduces Maxwell's radiation pressure in bulk, and Compton verified it photon by photon.
X-rays: the photoelectric effect in reverse
X-rays are made by accelerating electrons through – into a metal anode. Decelerating in the nuclear electric fields, they radiate a continuous spectrum — bremsstrahlung ("braking radiation") — plus sharp characteristic lines from shell transitions (P.2.2). Classically the continuum should extend to arbitrarily short wavelength; instead it stops dead at the Duane–Hunt cutoff. The photon explains it in one line: an electron arrives with kinetic energy , and the most energetic photon takes all of it in one quantum,
This is the photoelectric effect run backwards — electron in, photon out (, a few eV against tens of keV, is negligible). The cutoff depends only on , never on the anode material, and historically gave one of the cleanest measurements of ; with , , e.g. at . Meanwhile the same X-rays reflect off crystal planes with constructive interference at the Bragg condition — pure wave behavior, and the standard way X-ray wavelengths are measured. Hold that thought.
The Compton effect
Compton (1923) scattered X-rays off graphite and found scattered radiation at angle with a longer wavelength , shifted by an amount depending only on . A classical wave cannot do this — an electron driven at reradiates at — but a relativistic photon–electron collision can. Setup: a photon (, momentum along ) hits a free electron at rest; the photon exits at with wavelength , the electron at on the other side with momentum and energy . Energy, - and -momentum conservation give three equations:
Step 1 — eliminate . Isolate the electron terms in the momentum pair, square, add ():
Step 2 — eliminate . Isolate the square root in the energy equation and square:
Step 3 — equate. Multiply Step 1 by and set it equal to Step 2; the squared terms cancel, leaving . Multiply by :
The prefactor is the electron's Compton wavelength , so the shift runs from (forward) to (backscatter), independent of and of the material — exactly what Compton measured, with the recoil electron detected in coincidence with the scattered photon. In energy terms, with , the scattered photon has .
The unshifted peak. Compton also saw a component at the original : photons scattering off electrons so tightly bound that the whole atom recoils. Replace by the atomic mass and the shift shrinks by the same factor — unresolvably small.
Caution. Do not swap one cartoon for another: the photon is not a tiny billiard ball. The very same X-ray beam Bragg-diffracts off a crystal (wave) and Compton-scatters off its electrons (particle). No classical object does both; the resolution is that a quantum amplitude propagates like a wave and is detected like a particle — the formalism of P.3.2 and P.4.1.
Pair production and annihilation
Above roughly 1 MeV a new channel opens: the photon vanishes and an electron–positron pair appears, , with threshold set by the rest masses, . But this cannot happen in free space: each lepton has strictly (because ), so by the triangle inequality
i.e. the pair always has , while the photon has exactly — energy and momentum cannot both balance. Pair production therefore happens only near a nucleus, which absorbs the recoil momentum while (being heavy, ) carrying off negligible energy, leaving the threshold at . The time-reverse is annihilation: a slowed positron meets an electron essentially at rest, total momentum ; a single photon would carry — forbidden by the same argument — so annihilation at rest produces at least two photons, back-to-back with equal and opposite momenta, each (three-photon decay also occurs, from triplet positronium; two is the minimum). These back-to-back photon pairs are the working principle of PET imaging.
Worked Examples
Example 1 — Photoelectric effect on sodium
Sodium has ; shine light on it. Photon energy (with ): , so and . Threshold: , i.e. — green barely works, red does nothing. Doubling the intensity at 400 nm doubles the current; and do not move.
Example 2 — Compton scattering at 90°
Compton's beam, (Mo K), scattered at : , so . Energies: , ; cross-check with : . ✓ The recoil electron carries — small here, but MeV photons can hand the electron most of their energy (E5).
Hands-on (Python)
Fit synthetic stopping-potential data the way Millikan did — the slope of is for every metal; only the intercept changes.
import numpy as np
h_true = 6.62607015e-34 # Planck constant, J s
e = 1.602176634e-19 # elementary charge, C
rng = np.random.default_rng(7)
metals = {"Cs": 2.14, "Na": 2.28, "Zn": 4.33} # work functions phi, eV
for metal, phi in metals.items():
nu0 = phi * e / h_true # threshold frequency, Hz
nu = np.linspace(1.05 * nu0, 2.5 * nu0, 12) # measured frequencies, Hz
V0 = (h_true / e) * nu - phi # ideal line: slope h/e, intercept -phi/e
V0 += rng.normal(0.0, 0.02, V0.size) # 20 mV of measurement noise
slope, intercept = np.polyfit(nu, V0, 1) # least-squares straight line
print(f"{metal}: h = {slope * e:.3e} J s phi = {-intercept:.2f} eV")
# Expected output — h within ~1% of 6.626e-34 for every metal, e.g.:
# Cs: h = 6.645e-34 J s phi = 2.15 eV (Na, Zn similar; varies with the noise)Now the Compton kinematics: the wavelength shift is universal, but the energy lost depends strongly on the incident energy.
import numpy as np
import matplotlib.pyplot as plt
h, c, me = 6.62607015e-34, 2.99792458e8, 9.1093837015e-31
lam_C = h / (me * c) # Compton wavelength = 2.426e-12 m
mec2 = 0.51099895 # electron rest energy, MeV
theta = np.linspace(0.0, np.pi, 500)
fig, (ax1, ax2) = plt.subplots(1, 2, figsize=(10, 4))
ax1.plot(np.degrees(theta), lam_C * (1 - np.cos(theta)) * 1e12)
ax1.set(xlabel="θ (deg)", ylabel="Δλ (pm)", title="Compton shift")
# rises from 0 to 2*lam_C = 4.85 pm at 180°, independent of incident energy
for E in (0.1, 0.5, 1.0): # incident photon energies, MeV
ax2.plot(np.degrees(theta), E / (1 + (E / mec2) * (1 - np.cos(theta))), label=f"E = {E} MeV")
ax2.set(xlabel="θ (deg)", ylabel="E' (MeV)", title="scattered photon energy")
ax2.legend()
plt.tight_layout()
plt.show()
# At θ = 180° the 1 MeV curve drops to 1/(1 + 2·1.957) ≈ 0.20 MeV:
# harder photons lose a larger FRACTION of their energy to the electron.Exercises
E1 (easy). Cesium has . Can a helium–neon laser () eject photoelectrons from it at any intensity? Give the threshold wavelength.
Solution
: no single photon suffices, so no emission at any (ordinary) intensity — intensity only changes the photon rate. Threshold: ; anything redder fails.
E2 (easy). A 1.00 mW green laser pointer () shines on a black wall. Find the photon energy, the photons emitted per second, the momentum per photon, and the force on the wall.
Solution
; rate ; momentum ; force (full absorption) — equal to the classical , as it must be.
E3 (medium). Classical time-lag estimate: sodium () is illuminated at . If an atom of radius could only absorb the wave energy falling on its cross-section, how long until one electron accumulates ? Compare with experiment.
Solution
Collected power ; required energy ; time $t = 3.65\times10^{-19}/3.1\times10^{-26} = 1.2\times10^{7},\mathrm{s} \approx 135$ days. Observed lag: under a nanosecond. The energy is not spread over the wavefront — it arrives in quanta.
E4 (medium). Why did Compton need X-rays? Compute the maximum fractional shift for (a) green light, , and (b) Compton's X-rays, .
Solution
The maximum shift () is regardless of . (a) — buried below optical resolution and linewidth. (b) — easily resolved by Bragg spectrometry. The absolute shift is universal; only short wavelengths make it relatively visible.
E5 (hard). Derive the maximum kinetic energy the electron can gain in Compton scattering (the Compton edge), and evaluate it for a 511 keV photon.
Solution
The electron gains most when the photon backscatters, : with , , so . For , : . This sharp upper edge in the electron spectrum is a standard feature of gamma-ray detectors — the photon can never give a free electron all its energy (total absorption would violate the same -vs- bookkeeping as pair production in free space).
Checkpoint
- Which photoelectric facts contradict the classical wave picture, and how does explain each?
- What does the slope of Millikan's -vs- line measure, and why is it the same for all metals?
- Derive for the photon. Which relativistic ingredient makes it work?
- Why does Compton-scattered radiation contain an unshifted line as well as the shifted one?
- Why is pair production impossible in empty space, and why does annihilation at rest yield two photons, not one?
Answers
- Threshold frequency, no time lag, intensity-independence of , linear . Photons: one quantum per electron — below nothing works, energy arrives in a lump, intensity only sets the photon rate, and is linear by construction.
- The universal slope — nature's constants only; the metal enters solely via the intercept .
- From with : , so . The ingredient: a particle moving at must be massless.
- Some photons scatter off tightly bound electrons — effectively off the whole atom — so the shift with is unresolvably small.
- A pair always has while a photon has , so both conservation laws cannot hold without a nucleus taking recoil momentum. At rest the total momentum is zero, which one photon () cannot match — two back-to-back 511 keV photons can.
Further Reading
- [ER] Eisberg & Resnick, §2-2–2-4 — photoelectric effect, Einstein's quantum theory, and the Compton effect; the primary treatment this lesson follows.
- [ER] Eisberg & Resnick, §2-6–2-7 — X-ray production, pair production and annihilation.
- [Gri] Griffiths & Schroeter, §1.1–1.2 — where the story hands over to the wavefunction and the statistical interpretation.
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